Synchrotron and IC modelling of the radio halo (H) and relic (R) hosted by Coma. Caption as in Fig. 2. In the case of the relic, we do not show the line corresponding to Bdt because it gives worst estimates than that of BV. This is due to our assumption of uniform radio sources which is particularly inappropriate in case of objects with a large size in the sky, like Coma. See main text for details.
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